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20172021
most citedA stellar census in globular clusters with MUSE: The contribution of rotation to cluster dynamics studied with 200 000 stars

220 citations · 817 across the 15 of their papers we have counts for

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Showing 2018Show all

5 papers · 1 filter

astro-ph.GA2018★ 61 cited

Cluster kinematics and stellar rotation in NGC 419 with MUSE and adaptive optics

Sebastian Kamann, Nathan J. Bastian, Tim-Oliver Husser +9

We present adaptive optics (AO) assisted integral-field spectroscopy of the intermediate-age star cluster NGC 419 in the Small Magellanic Cloud. By investigating the cluster dynami…

astro-ph.GA2018★ 46 cited

MUSE crowded field 3D spectroscopy in NGC300 I. First results from central fields

M. M. Roth, C. Sandin, S. Kamann +9

Aims. As a new approach to the study of resolved stellar populations in nearby galaxies, our goal is to demonstrate in NGC300 that integral field spectroscopy with high spatial res…

astro-ph.GA2018★ 75 cited

A 3.5-million Solar Masses Black Hole in the Centre of the Ultracompact Dwarf Galaxy Fornax UCD3

Anton V. Afanasiev, Igor V. Chilingarian, Steffen Mieske +16

The origin of ultracompact dwarfs (UCDs), a class of compact stellar systems discovered two decades ago, still remains a matter of debate. Recent discoveries of central supermassiv…

astro-ph.GA2018★ 38 cited

Upper limits on the presence of central massive black holes in two ultra-compact dwarf galaxies in Centaurus A

Karina T. Voggel, Anil C. Seth, Nadine Neumayer +10

The recent discovery of massive black holes (BHs) in the centers of high-mass ultra compact dwarf galaxies (UCDs) suggests that at least some are the stripped nuclear star clusters…

astro-ph.GA2018★ 47 cited

Climbing to the top of the galactic mass ladder: evidence for frequent prolate-like rotation among the most massive galaxies

Davor Krajnovic, Eric Emsellem, Mark den Brok +4

We present the stellar velocity maps of 25 massive early type galaxies located in dense environments observed with MUSE. Galaxies are selected to be brighter than M_K=-25.7 magnitu…